UPK 185
0.84
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
40.3 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 185 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 346.411 | 49.377 | 1.794 | 2.641 | -1.955 | -11.024 |
| Li et al. | 2025 | 346.424 | 49.376 | 1.786 | 2.636 | -1.929 | â |
| Almeida et al. | 2025 | 346.356 | 49.36 | â | â | â | â |
| Alfonso et al. | 2024 | -13.559 | 49.38 | 1.771 | 2.64 | -1.95 | â |
| Zhang et al. | 2024 | 346.408 | 49.367 | â | â | â | â |
| Hunt & Reffert | 2024 | 346.408 | 49.367 | 1.789 | 2.646 | -1.933 | -12.297 |
| Cavallo et al. | 2024 | 346.465 | 49.386 | 1.791 | â | â | â |
| Hunt & Reffert | 2023 | 346.408 | 49.367 | 1.789 | 2.646 | -1.933 | -12.297 |
| He et al. | 2022 | 346.427 | 49.392 | 1.796 | 2.642 | -1.955 | â |
| Tarricq et al. | 2022 | 346.448 | 49.405 | 1.79 | 2.633 | -2.005 | â |
| Dias et al. | 2021 | 346.356 | 49.36 | 1.788 | 2.639 | -1.935 | -10.817 |
| Cantat-Gaudin et al. | 2020 | 346.424 | 49.376 | 1.786 | 2.636 | -1.929 | â |
| Cantat-Gaudin & Anders | 2020 | 346.437 | 49.377 | 1.784 | 2.641 | -1.919 | â |
| Sim et al. | 2019 | 346.428 | 49.377 | â | 2.66 | -1.93 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.55 | 0.44 | 0.76 | 97 | 0.116 | 228 | â | â |
| Li et al. | 2025 | 0.54 | 0.43 | â | 97 | 0.030 | â | â | â |
| Almeida et al. | 2025 | 0.55 | 0.43 | â | 219 | â | 210 | â | â |
| Alfonso et al. | 2024 | 0.57 | 0.45 | â | 97 | 0.116 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.066(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 246(1) | â | â |
| Cavallo et al. | 2024 | 0.57 | 0.60 | â | 105 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 0.53 | 0.27 | 0.76 | 129 | â | â | â | â |
| He et al. | 2022 | â | 0.50 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.56 | â | â | 74 | â | â | â | â |
| Dias et al. | 2021 | 0.55 | 0.43 | â | 219 | 0.117 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.57 | 0.45 | â | 71 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.55 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.55 | â | â | 89 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.